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Phys. Rev. C 74, 054303 (2006) [9 pages]

Shell model method for Gamow-Teller transitions in heavy, deformed nuclei

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Zao-Chun Gao1,2,3, Yang Sun1, and Y.-S. Chen3,4
1Joint Institute for Nuclear Astrophysics and Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA
2Department of Physics and Astronomy and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
3China Institute of Atomic Energy, P.O. Box 275(18), Beijing 102413, People's Republic of China
4Institute of Theoretical Physics, Academia Sinica, Beijing 100080, People's Republic of China

Received 24 May 2006; published 8 November 2006

A method for calculation of Gamow-Teller transition rates is developed by using the concept of the Projected Shell Model (PSM). The shell model basis is constructed by superimposing angular-momentum-projected multiquasiparticle configurations, and nuclear wave functions are obtained by diagonalizing the two-body interactions in these projected states. Calculation of transition matrix elements in the PSM framework is discussed in detail, and the effects caused by the Gamow-Teller residual forces and by configuration-mixing are studied. With this method, it may become possible to perform a state-by-state calculation for β-decay and electron-capture rates in heavy, deformed nuclei at finite temperatures. Our first example indicates that, while experimentally known Gamow-Teller transition rates from the ground state of the parent nucleus are reproduced, stronger transitions from some low-lying excited states are predicted to occur, which may considerably enhance the total decay rates once these nuclei are exposed to hot stellar environments.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.74.054303
DOI:
10.1103/PhysRevC.74.054303
PACS:
21.60.Cs, 23.40.Hc, 23.40.Bw